VSAT SATOM TRAINING
Course Introduction
Welcome to the VSAT Installer Training Course. We have put together a comprehensive course that covers all aspects of the VSAT field technician. By the end of the course, we hope you are confident with the installation, operation, maintenance, and fault finding of VSAT satellite equipment.
Here are a few tips to help you during the course:
- Take your time during the lessons.
- Take notes.
- Go back and re-read the lesson if needed.
- If you don’t understand, email satoms support.
- Download the PDF help sheets, software, manuals, spec sheets, and course notes for future reference.
- Enjoy!
Email support@satoms.com if you have any questions during the course. Please remember to leave a course review when you have finished!
Click the ‘Complete’ button below at the end of a lesson to mark it as completed in your user account.
What is VSAT?
VSAT is used in remote areas of the world. A connection to the traditional copper or fiber network is impossible or is used as a backup communication link for mission-critical systems. VSAT is an acronym for Very Small Aperture Terminal and generally refers to a satellite antenna less than 3.8m located at the remote site. VSAT is used for two-way communication for voice and data traffic.
Geostationary communication satellites are positioned one-tenth of the way to the moon (about 36,000 km) and appear stationary when viewed from the Earth’s surface. Many service providers use Geostationary satellites because a fixed antenna can be used and are relatively inexpensive. For Medium Earth Orbit (MEO) satellites, like the O3B network or satellites in an inclined orbit, tracking antennas must be used. These will be covered later in the course.
This video by SES shows how satellites stay in orbit and how VSAT works.
Frequency Bands
Satellite VSAT communication is split into four Radio Frequency (RF) bands within which commercial communication and military satellites operate. These different frequency bands have separate uplink (Transmit) and downlink (Receive) frequencies, require different RF components (LNB and BUC), and are suited to different applications. Commercial satellite service providers use C Band, Ku Band, and occasionally Ka-Band.
C Band
uplink 5.925 – 6.425 GHz
downlink 3.7 – 4.2 GHz
The C band is primarily used for voice and data communications. Because of its weaker power requires a larger antenna, usually above 1.8m (6ft). However, due to the lower frequency range, it performs better under adverse weather conditions like rain.
X Band
uplink 7.9 – 8.4 GHz
downlink 7.25 – 7.75 GHz
The X band is used mainly for military communications and Wideband Global SATCOM (WGS) systems and is not used commercially. With relatively few satellites operating in the X band, there is a wider separation between adjacent satellites, making it ideal for Comms-on-the Move (COTM) applications. This band is less susceptible to rain fade than the Ku Band due to the lower frequency range, resulting in a higher performance level under adverse weather conditions.
Ku Band
uplink 14 – 14.5GHz
downlink 10.9 – 12.75 GHz
Ku (K band Under) band is typically used for commercial VSAT systems. Example uses include offshore oil & gas, maritime, and land-based enterprise connectivity. The antenna sizes, ranging from 0.9m -1.8m (~6ft), are much smaller than the C band because the higher frequency means that higher gain can be achieved with small antenna sizes than C band. Networks in this band are more susceptible to rain fade, especially in tropical areas, and Adaptive Coding Modulation (ACM) is used to prevent these outages.
Ka-Band
uplink 26.5 – 40 GHz
downlink 18 – 20 GHz
The Ka-band (K band Above) is primarily used for two-way consumer broadband and military networks. Ka-band dishes can be much smaller and typically range from 60cm-1.2m (2′ to 4′) in diameter. Transmission power is much greater compared to the C, X, or Ku band beams. This band’s higher frequencies can be more vulnerable to signal quality problems caused by rain fade. Again ACM is used to help rain fade. O3b Network satellite service uses Ka-Band for its connectivity.
Satellite Orbits
A communications satellite is a satellite located in space for telecommunications. There are three altitude classifications for satellite orbits.
LEO – Low Earth Orbit
LEO satellites orbit from 160-2000km above the earth, take approximately 1.5 hrs for a full orbit, and only cover a portion of the earth’s surface, therefore requiring a network or constellation of satellites to provide global, continual coverage. Due to the proximity to Earth, LEO satellites have a lower latency (latency is when a packet is transmitted and the moment it reaches its destination) and require less amplification for transmission.
MEO – Medium Earth Orbit
MEO satellites are located above LEO and below GEO satellites and typically travel in an elliptical orbit over the North and South Pole or in an equatorial orbit. These satellites are traditionally used for GPS navigation systems and are sometimes used by satellite operators for voice and data communications. MEO satellites require a constellation of satellites to provide continuous coverage. Tracking antennas are needed to maintain the link as satellites move in and out of the antenna range.
GEO – Geostationary Orbit
GEO satellites orbit at 35,786 km (22,282 mi) above the equator in the same direction and speed as the earth rotates on its axis. This makes it appear to the earth station as fixed in the sky. Most commercial communications satellites operate in this orbit; however, there is a longer latency due to the earth’s distance.
VSAT Link Terminology
VSAT terminology can often be confusing at first, but it’s really quite simple, and this diagram shows how it relates to the VSAT remote site or the Teleport hub side.
The Uplink is always the link to the satellite, and the downlink is always the link from the satellite irrespective of which side of the link you are, Teleport/Hub or VSAT remote site.
Inbound and Outbound are often referred to as Inroute(s) and Outroute(s). The Outbound is from the teleport hub to the remote VSAT, and the Inbound is the remote VSAT to the teleport hub.
VSAT Latency
A satellite VSAT link’s latency time is a crucial factor when choosing to use a satellite system. It can affect your network’s performance, and some applications experience issues when the latency is too high, not to mention a poor user experience.
Radio Frequency (RF) waves travel at the speed of light, which is a little less than 300,000 km per second (299,792.458 km/s). We can calculate how long a signal will travel from the antenna to the satellite and back down to the distant end of the link. The latency is unaffected by the frequency band of the link.
But not all satellites were created equal. Depending on the type of orbit (i.e., distance) of the satellite, travel time will vary.
VSAT Latency Calculation
We can use the simple speed, distance, and time equation to calculate the time:
speed = distance / time
time = distance / speed
A Geo VSAT Satellite Example
time = 35,786 km / 299,792 km/s
time to satellite = 0.11937 seconds
Therefore, the RF signal’s time to reach the satellite is 0.11937 seconds, but we must come back down again, so it’s really 0.23874 sec or approx. 0.25 sec for a signal (or information, data, packet) to travel across a satellite link. This is called one ‘hop’.
TCP applications (like Pings, internet browsing) require an ‘ack,’ and the Return Trip Time (RTT) of a VSAT link is just under 0.5 seconds or 500 msec.
VSAT Latency Times (PING)
Acceptable latency times over a VSAT link are between 550 – 750 msec. This is more than the 500 msec return trip time due to the data packet processing by the VSAT router, Teleport equipment, etc.
A ping to a device at the other end of the link should be used to get a true reading of the satellite latency, i.e., the distant VSAT modem or hub, Teleport router, or switch. To find a suitable device, you can perform a traceroute to google, showing the route’s connected equipment. Pick a device just after the satellite link. Check the latency times!
If the ping time of the link is greater than 900 msec, we need to consider what other factors might be causing the additional time.
These might include some of the following:
- Traffic congestion – The local traffic is demand is much greater than your VSAT bandwidth.
- Terrestrial links – What route is your traffic taking to reach the destination
- Server location and load – The ping server might be under load and running at max CPU usage
- Distant end equipment
- Oversubscribed VSAT network – the most common cause of VSAT satellite latency, and you need to speak with your satellite provider!
Reducing VSAT Latency
The latency time can be reduced by:
- Using an MEO satellite service like O3B
- Reduce local traffic like software updates – schedule when the office is unattended
- Reduce unwanted traffic on the link like social networks, video downloads, and bittorrents
- Ensure there is adequate network bandwidth available and the service is not oversubscribed.
- Traceroute to google to check where the issue is
- Ping a device at the distant end (Teleport)
VSAT satellite latency should be between 550 and 750msec on a good link.
Rain Fade
Rain fade is the deterioration of the microwave RF signal levels caused by rain precipitation on either end of the satellite VSAT link. Typically, Ku and Ka-band links are affected (frequencies above 11GHz) and can occur at the VSAT remote or the link’s Teleport end. RF energy is absorbed and scattered by the rain droplets and affects the higher frequencies more because of the signal’s wavelength and the size of the rain and the droplet’s shape. Cross polarization isolation will also be reduced.
Line of Sight
Rainstorms many km away from the antenna could still have a detrimental effect, especially if the elevation angle is quite low. The storm is in the line of sight of the antenna and can last for prolonged periods.
VSAT Antenna
Water, snow, and Ice on the antenna and RF feed assembly surface will also cause a decrease in signal levels by approx. 5-15%. A Radome will protect the VSAT electronics from the weather and corrosion, but the water on the Radome’s surface will attenuate the signal when it rains.
Clouds
Clouds are made from water vapor, causing significant loss on high-frequency satellite links. The typical attenuation at Zenith (0° Elevation) is only a few dB below 100 GHz.
Rain Fade Solutions
Possible ways to overcome the effects of rain fade are;
- Site diversity
- Satellite diversity
- Uplink Power Control (UPC)
- Adaptive Coding and Modulation (ACM)
- Hydrophobic coatings on the antenna or Radome
- C-Band VSAT communications
- Link budgets
- Antenna heated blankets
Sun Outage or Solar Transit Events
What is a Sun Outage?
A sun outage (or a solar transit event or sun fade) happens twice a year during the equinox in March and September, when the Sun is directly above the Equator. Each outage lasts for several minutes for a few days and is caused by the satellite passing directly in front of the Sun as the Earth rotates.
The antenna can see the Sun behind the satellite for these short periods, and the LNB receiver is briefly overwhelmed with RF energy (noise) from the Sun. The link’s noise floor will be increased, swamping out the satellite signal for a few minutes. This might cause a total outage of communications or poor throughput depending on the link’s robustness (MODCOD, power). All frequency bands experience increased RF noise during these periods.
Larger dishes (normally at the teleport/hub end) have a narrower, more focused beam and experience shorter outage periods, repeating over a shorter number of days than smaller antennas. But an outage of the hub antenna will affect multiple customers, while an outage at the remote VSAT antenna only affects the link on that antenna.
So, this means each VSAT communication link will experience two sun outages per equinox.
A 2.4m C-band dish will typically see about 11-minute outages daily, recurring at the same time
over the course of a week. The outage time will peak in the middle of the outage cycle.
How to calculate your outages
Several websites can calculate sun outages’ timings, such as this tool, with the antenna locations, frequency band, and size for both antennas.
Adaptive Coding Modulation (ACM)
Adaptive Coding and Modulation (ACM) is a technology that automatically changes the Forward Error Correction (FEC) and modulation utilized on a satellite link to compensate for changes in link conditions to operate at the most efficient coding and modulation scheme available.
Why use ACM?
The changes in link performance are commonly due to atmospheric conditions like rain (rain fade), changes in the RF levels, solar events, noise, or interference. Previously these conditions could result in the link dropping out of the network and making the users angry. ACM prevents these outages and will provide a more robust service, and the link will only drop out under extreme conditions.
- More robust link
- Maximizes link availability
- Required to meet SLA (Service Level Agreements)
- More spectrally efficient for the outbound carrier and remote sites – more data bits per Hz
- MODCOD automatically altered per remote link
- Happy Satellite VSAT users 😊
How does ACM Work?
ACM evaluates current link conditions and throughput requirements through a return channel to determine the ideal modulation and FEC used (MODCOD). This optimizes the bandwidth efficiency for maximum throughput on a remote-by-remote basis in real-time without any intervention from the Network Operations Centre (NOC). The ACM can be limited at a set MODCOD (e.g., 16APSK) to stop any CRC errors if the remote is incapable of receiving these higher-level MODCODs in clear sky conditions.
Linear Polarization
When installing VSAT satellite equipment, you will need to know what polarization is used on the link, and you will have to set up the RF feed assembly correctly.
Cross-Pol (or XPOL) and Co-Pol are used for linear VSAT links.
What do Xpol and Co-Pol mean?
Cross-Pol or XPOL is when the transmit and receive RF signals are separated by 90 degrees. So, when the transmit is vertical, the receive will be horizontal and vice versa.
- Rx vertical and Tx horizontal
- Rx horizontal and Tx vertical
Co-Pol is when the transmit and receive signals are both on the same plane. Transmit and receive are both vertical or horizontal.
- Rx vertical and Tx vertical
- Rx horizontal and Tx horizontal
VSAT Link Commissioning
The satellite operator will normally require you to rotate the RF feed horn to achieve at least 30dB of isolation during the commissioning process. This test is called CPI (Cross Polarisation Isolation). This reduces the interference of your transmit signal on the opposite polarization that might be used by someone else. The NOC (Network Operations Centre) will set up a conference call with the satellite operator. After setting up a Continuous Wave (CW) transmission, you will be asked to move the RF feed horn by 1 or 2-degree steps in one direction and then in the opposite direction. The satellite operator will be looking at both pols on a spectrum analyzer and measuring the max isolation. You may be asked to peak the antenna in azimuth and elevation.
The tech moves the RF feed assembly by hand for static land-based sites and locks it into position after commissioning. Stabilized antennas (SeaTel, Intellian, and SpaceTrack) have an auto-pol motor to move the feed assembly during normal operation. During the commissioning, this has to be disabled and adjusted from the ACU. More details on how to do this are included in the SeaTel and Intellian courses.
With lengthy commissioning testing, some modems will sometimes timeout (safety feature to prevent CW being left on), and you will have to hit ‘Start CW’ again.
After the satellite operator is finished the testing, the results should be recorded for future reference. The remote compression point (1dB point) will normally be checked during this process.
So, achieving good isolation is very important. If this is not done, you will cause interference on the network. The transmit power will be high (reducing the fade margin), lower link MODCOD and the remote site’s inferior performance. It’s best practice to set the polarisation correctly the first time.
RF Equipment
Identifying the correct parts is a massive help. Many people have wasted considerable time and effort only to determine that the incorrect parts have been fitted to the RF feed assembly. If you have inherited equipment from a previous service provider, knowing if it will work quickly will save you time and money.
Cross-Pol combiner the transmit and receive ports are at right angles to each other.
Co-Pol combiner the waveguide ports are in the same direction.
How to calculate and set up the RF feed assembly’s polarization angle to be covered in more detail later in the course.
Circular Polarization
The circular polarization of an electromagnetic wave is a polarization state in which, at each point, the electric field of the wave has a constant magnitude. Still, its direction rotates with time at a steady rate in a plane perpendicular to the wave’s direction.
Circular polarization may be referred to as right-handed or left-handed, clockwise or anti-clockwise, depending on the electric field vector rotates’ direction. Unfortunately, two opposing historical conventions exist, so always check if the polarization is from the signal source or the receiving dish.
Circular polarization can either be RHCP or LHCP.
RHCP – Right Hand Circular Polarization
LHCP – Left Hand Circular Polarization
Link Commissioning
There should be no need to adjust the RF feed assembly’s polarization as the Tx and Rx are circularised on the feed; however, the satellite operator may still want to check the isolation. Cheaper circularises are not precisely circular and more of an oval shape, and you might have to rotate it to achieve isolation.
deciBels (dB)
If you are working in satellite or communications, you will often use dB’s. But what are they?
Bels are too big, so we use deciBels (dB). These are easy ways to multiply large and small numbers. By using dBs, you can add or subtract instead of having to multiply numbers. DBs is a ratio between two levels, and an example is the received signal to noise level (Rx SNR) expressed in dBm (this tells us how strong the signal level is compared to the noise with reference to 1mW).
dB = 10 log [ratio of two power levels]
deciBel (dB) | Power |
+10dB | x 10 |
+3dB | x 2 |
0dB | x 1 |
-3dB | x 0.5 |
-10dB | x 0.1 |
Question: A 30m RG6 coax has a loss of 3dB. What is the output power if the input is 500mW?
dBW or dBm?
dBW is referenced the power with 1W (Watt)
dBW | Power |
20dBW | 100 Watts |
10dBW | 10 Watts |
3dBW | 2 Watts |
0dBW | 1 Watt |
-3dBW | 0.5 Watts |
-30dBW | 0.001 Watts |
dBm is reference the power with 1mW (milliWatt)
dBm | Power |
20dBm | 100 mW |
10dBm | 10 mW |
3dBm | 2 mW |
0dBm | 1 mW |
-3dBm | 0.5 mW |
-30dBm | 0.001 mW |
dBm to dBW Conversion
The conversion between dBm and dBW is quite straightforward. 1 Watt is equal to 1000mW, which is an increase of 30dB. So we need to add or subtract 30dB.
dBm = dBW + 30dBW = dBm – 30
Example: Convert 35dBm to dBW
Example: Convert -40dBW to dBm
- Using decibels (dB), you can quickly calculate the overall gain of a communication system by simply adding or subtracting the different components.
DC Voltages
WARNING!
DC Voltages can be supplied by the modem on the Rx and Tx coax connectors. Care must be taken when connecting and disconnecting to prevent equipment damage.
The modem supplies DC voltage for the LNB RX (19V) and BUC TX (24 or 48V) on the coax connector’s center pin.
Care must be taken not to short out this pin when the modem is powered up. Don’t let the center pin touch anything metal if the modem is powered up.
It’s recommended that the modem is powered down when connecting the coax at either end.
Comments
Post a Comment